Revista Mexicana de Astronomía y Astrofísica ISSN: 0185-1101 [email protected] Instituto de Astronomía México

García López, R. J.; the MAGIC Collaboration SEARCH FOR GAMMA-RAY EMISSION FROM THE REMNANT IC 443 WITH THE MAGIC TELESCOPE Revista Mexicana de Astronomía y Astrofísica, vol. 35, junio, 2009, pp. 62-63 Instituto de Astronomía Distrito Federal, México

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How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative © 2009: Instituto de Astronomía, UNAM - 12th IAU Regional Latin American Meeting of Astronomy Ed. G. Magris, G. Bruzual, & L. Carigi b b In the gaining v E what cles prop isotopically cating resem lativistic Based equals MA to Earth. T pairs, tivit strategy Siguiendo Av. fuen Key nismo related para T estar 38205 Observ R 62 elo enerife, e e eV evMexAA − das 3 2 1 this efficien 2 scattered Up Cosmic http://wwwmagic.mppmu.mpg.de/ Departamen Instituto 1. GIC. . cit ? y te Wor (99%). 2 ortional Astrof observ el , La relacionados bles are can INTR SEAR y resp los the on de aciones whic to a scenario, that . telescopio to F momen Spain. 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G. Magris, G. Bruzual, & L. Carigi acceleration MHz F line radio previously energy with SNR mass the the pheric ging timal Fig. cen surface 0.05 w a lection, and in analysis de under nergy P the urthermore, alma as Decem ter los ) The A sp end other additional 1. supp deg corresp Cerenk ( 45 (p maser ectrum and first efficiency threshold ∼ of construction (a) Muc (Canary 2. imaging (VHE) (PWN) ossibilit 0 of it 2 MA of 10 sho the b osed diameter, region OBSER X can hand, Distribution 236 er 2008. for observing 4 hac onding GIC o w emission ra source M exp of v) 2005–Jan ed there detect this ys to 40 hos m

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